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The gamma-ray emitting microquasar LSI+61303
M. Massi, M. Ribo', J. M. Paredes +3
LS I +61 303 is one of the most studied X-ray binary systems because of its two peculiarities: On the one hand being the probable counterpart of the variable gamma ray source 2CG 1…
Radio-loud and Radio-quiet X-ray Binaries: LSI+61303 in Context
Maria Massi
The three basic ingredients - a spinning compact object, an accretion disc and a collimated relativistic jet - make microquasars a galactic scaled-down version of the radio-loud AG…
LSI+61303 in the context of microquasars
Maria Massi
LSI+61303 is one of the most observed Be/X-ray binary systems because, peculiarly, it has periodical radio and X-ray emission together with strong, variable gamma-ray emission. Thi…
EVN and MERLIN observations of microquasar candidates at low galactic latitudes
M. Ribo, E. Ros, J. M. Paredes +2
In an attempt to increase the number of known microquasars, Paredes et al. (2002) have presented a long-term project focused on the search for new objects of this type. They perfor…